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The rotational deformations of two kinds of neutron stars are calculated by using Hartle‘s slow-rotation formulism. The results show that only the faster rotating neutron star gives an obvious deformation. For the slow rotating neutron star with a period larger than hundreds of millisecond, the rotating deformation is very weak. 相似文献
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Unified Understanding of Giant Magnetoresistance Effect and Magnetization in Granular Films with Two-Particle Size Distribution 下载免费PDF全文
Jian-QingWANG JordanPeck FinnobarrO'Grady NamKim 《中国物理快报》2004,21(11):2255-2258
The giant magnetoresistance (GMR) effect and magnetization curves of Cu80 Co20 granular thin films are studied and measured in a superparamagnetism temperature (180K). The correlation between the GMR effect and the magnetization is analysed in a unified framework. These two independent properties are fitted by assuming that there are two size distributions in the Co nano-particle population. Under an assumption, good fittings are achieved for both the GMR and the magnetization, using the minimal number of parameters. The obtained average particle sizes for the smaller and larger particles are 1.0hm and 2.8nm, respectively. In fitting the magneto-transport, a power scaling relationship with the particle size for each size population is proposed, and the fitted results reveal that a certain degree of magnetic bulk scattering is present in larger particles. 相似文献
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Effect of the Quadrupole Moment of a Rotating Massive Object on the Gravitational Faraday Rotation 下载免费PDF全文
We study the rotation of the polarization plane for a ray of electromagnetic radiation propagating in the gravitoelectromagnetic field caused by a rotating massive object with the quadrupole moment.The effect of the quadrupole moment on the gravitational Faraday rotation is investigated.It is found that the gravitational Faraday effect of the quadrupole moment is negligible for Kerr black holes,but this effect is important for rapidly rotating neutron stars. 相似文献
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ZuoWei 《近代物理研究所和兰州重离子加速器实验室年报》2003,(1):4-4
The equation of state (EOS) of spin-polarized nuclear matter has been investigated within the spin-dependent; Brueckner-Hartree-Fock framework by adopting the realistic nucleon-nucleon interaction supplemented with a microscopic three-body force. The three-body force effects have been studied and stressed with a special attention. The calculated results are given in Fig.1. It is seen that; in the Brueckner-Hartree-Fock framework the predicted energy per particle of spin-polarized nuclear matter versus the neutron and proton spin-polarization parameters fulfills a quadratic law in the whole range of spin-polarization. The related physical quantities such as spin the Landau parameters Go in spin channel and G′0 in spin-isospin channel, have been also calculated. 相似文献
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地球自身的旋转轴经受着多种旋转力的作用,例如二分点(即旋转轴处于春分、秋分点时)的进动等.最近发现有两个重要的旋转运动不被人注意地相互间抵消了.比利时的地球物理学家S.Lambert博士精确地测量到了这类在常规下是很难探测到的微弱晃动.这两个晃动分别是现在还不太明白其起因的钱德勒章动(Chandler wobble),这个章动的周期是433天.另一个是起源于地球上气候变化引起的晃动.这两个运动的综合后果应该导致地轴发生大于10米的移动.但由于这两个晃动的相互抵消作用,从2005年12月到2006年2月这段时间,地轴的移动却降低到了1米以下. 相似文献
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以二维旋转简谐振子势为例分析了在BEC中经常用到的旋转势,分析了哈密顿量的表达式,给出了波函数和能量本征值,并注意到了二维旋转简谐振子势与带电粒子在磁场中的情形具有相近的形式. 相似文献
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